Table B.1.
Slope of the MZR in various observational samples and in simulations.
| Study | Redshift | [log(M★/M⊙)] | γ | Znorm | Description |
|---|---|---|---|---|---|
| This work (direct-Te) | 6.3-7 | [6.89, 10.54] | 0.12 ± 0.08 | 7.96 ± 0.10 | f[O III]λ5008 selected galaxies from NIRCam/WFSS (EIGER, COLA1 and ALT surveys) |
| Greenpeas (Yang et al. 2017a) and Blueberries (Yang et al. 2017b) | z < 0.2 | [6.6,9.84] | 0.17 ± 0.01 | 8.19 ± 0.03 | Analogues for high-z galaxies because of their compact size, high equivalent width emission lines, high ionisation parameters and low metallicities. |
| Scholte et al. (2024)a | < 0.6 | [6.4, 11.05] | 0.23 ± 0.003 | 8.70 ± 0.003 | Sample from the DESI BGS validation and Year 1 Main Survey Data (Hahn et al. 2023) |
| Sanders et al. (2021) | ∼0.08 | [8.5, 11.5] | 0.28 ± 0.01 | 8.77 ± 0.01 | z ∼ 0 sample from SDSS (York et al. 2000, Andrews & Martini 2013). |
| 2.3 | [9.3, 10.7] | 0.30 ± 0.02 | 8.51 ± 0.02 | z ∼ 2 − 3 star-forming galaxies from MOSDEF survey (Kriek et al. 2015). | |
| 3.3 | [9.2, 10.6] | 0.29 ± 0.02 | 8.41 ± 0.03 | ||
| Li et al. (2023) | ∼2 | [6.52, 9.45] | 0.13 ± 0.04 | 8.31 ± 0.04 | JWST/NIRISS slitless grism spectroscopic observations in the Abell 2744 and SMACS J0723-3732 fields. |
| ∼3 | [7.39, 9.68] | 0.16 ± 0.03 | 8.24 ± 0.03 | Uses the O32 calibration from Bian et al. (2018). | |
| He et al. (2024) | 1.90 | [6.9, 9.9) | 0.223 ± 0.017 | 8.569 ± 0.036 | JWST/NIRISS slitless grism spectroscopic observations in the Abell 2744 field. |
| 2.88 | [7.1, 10.0) | 0.294 ± 0.010 | 8.596 ± 0.024 | Uses calibrations from Bian et al. (2018). | |
| Nakajima et al. (2023) | 4 − 10 | [7.39, 9.48] | 0.25 ± 0.03 | 8.24 ± 0.05 | JWST/NIRSpec data from ERO, GLASS and CEERS programmes |
| Curti et al. (2024) | 3 − 10 | [6, 10] | 0.17 ± 0.03 | 8.06 ± 0.18 | JWST/NIRSpec MSA data from the JADES programme. |
| 3 − 6 | [6, 10] | 0.18 ± 0.03 | 8.11 ± 0.03 | Uses calibrations from | |
| 6 − 10 | [6, 10] | 0.11 ± 0.05 | 7.87 ± 0.06 | Curti et al. (2020) | |
| Chemerynska et al. (2024) | ∼7 | [5.80, 7.19] | 0.39 ± 0.02 | 8.42 ± 0.17 | JWST/NIRSpec low-resolution Prism spectra from UNCOVER Survey. |
| Chakraborty et al. (2025) | 3 − 10 | [7.5, 10] | 0.21 ± 0.03 | 7.99 ± 0.21 | JWST/NIRSpec data |
| Li et al. (2025) | ∼6 | [7.44, 8.84] | 0.26 ± 0.01 | 8.00 ± 0.01 | f[O III]λ5008 selected galaxies from NIRCam/WFSS (ASPIRE and EIGER surveys) |
| SPHINX20(No selection cut) | 5 − 7 | [6.51, 10.46] | 0.41 | 8.10 | Hydrodynamical simulation |
| (With selection cut) | 5 − 7 | [8.46, 10.46] | 0.22 | 7.86 | |
| FLARESb (No selection cut) | 5 − 7 | [8.0, 11.31] | 0.44 | 8.25 | Hydrodynamical simulation |
| (With selection cut) | 5 − 7 | [8.0, 11.31] | 0.44 | 8.25 | |
| JAGUAR (No selection cut) | 5 − 7 | [5.98, 9.96] | 0.24 | 8.41 | Catalogue from empirical relations |
| (With selection cut) | 5 − 7 | [6.86, 9.96] | 0.10 | 8.27 | |
Notes. (a)Eq. 4 fit to data below turnover mass. (b)Eq. 4 fit to 50th percentile of the mass-weighted gas-phase metallicity.
References. (1) SPHINX20 (Katz et al. 2023); (2)FLARES (Lovell et al. 2020; Vijayan et al. 2020); (3) JAGUAR catalogue (Williams et al. 2018);
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